Abstract
A spatially-homogeneous and anisotropic-cosmological model in a scalar-tensor theory proposed by Sen and Dunn (1971) is obtained when the source of the gravitational field is a perfect fluid with pressure equal to energy density and the metric is of Bianchi type-I. Various physical properties of the model have also been discussed.
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Reddy, D.R.K., Venkateswarlu, R. An anisotropic cosmological model in a scalar-tensor theory of gravitation. Astrophys Space Sci 135, 287–290 (1987). https://doi.org/10.1007/BF00641564
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DOI: https://doi.org/10.1007/BF00641564